We report the first optical and control performances of the Tor Vergata Fabry-P´erot interferometer prototype designed and realized in the framework of the ADvanced Astronomy for HELIophysics (ADAHELI) solar mission project. The characterization of the the coated surfaces of the two plates defining the optical cavity has been carried out with a Zygo interferometer able to measure the microroughness and global curvature of the cavity. The peak-to-valley errors are compliant with the manufacturer specifications and correspond to λ/70 and λ/80 @632.8 nm respectively. In addition, we present a first estimate of the interferometer spectral stability in stable open-air condition. A spectral uncertainty equal to 0.95 pm is found as the typical RMS...
International audienceThe sensitivity of interferometric gravitational wave detectors is optimized, ...
A tunable Fabry-Perot interferometer (FPI) can be used as an optical band-pass filter. This type of ...
The sensitivity of interferometric gravitational wave detectors is optimized, in part, by balanced f...
We report the first optical and control performances of the Tor Vergata Fabry-P´erot interferometer ...
In this contribution we present preliminary mechanical and optical tests of the Fabry-Ṕerot interfer...
ADAHELI ADvanced Astronomy for HELIophysics is a solar satellite designed to investigate the fast dy...
Aims. Properly characterizing Fabry-Perot interferometers (FPI) is essential for determining their e...
Large Fabry-Pérot Interferometers (FPIs) are used in a variety of astronomical instrumentation, incl...
This contribution follows up with project Interferometry with compensation of the refractive index o...
Abstract The Fabry-Pérot interferometer is used in a variety of high-precision optical interferometr...
The interferometric gravitational wave detector Virgo has successfully completed the first major ste...
A non-Gaussian, flat-top laser beam profile, also called Mesa Beam Profile, supported by non spheric...
International audienceThe sensitivity of interferometric gravitational wave detectors is optimized, ...
A tunable Fabry-Perot interferometer (FPI) can be used as an optical band-pass filter. This type of ...
The sensitivity of interferometric gravitational wave detectors is optimized, in part, by balanced f...
We report the first optical and control performances of the Tor Vergata Fabry-P´erot interferometer ...
In this contribution we present preliminary mechanical and optical tests of the Fabry-Ṕerot interfer...
ADAHELI ADvanced Astronomy for HELIophysics is a solar satellite designed to investigate the fast dy...
Aims. Properly characterizing Fabry-Perot interferometers (FPI) is essential for determining their e...
Large Fabry-Pérot Interferometers (FPIs) are used in a variety of astronomical instrumentation, incl...
This contribution follows up with project Interferometry with compensation of the refractive index o...
Abstract The Fabry-Pérot interferometer is used in a variety of high-precision optical interferometr...
The interferometric gravitational wave detector Virgo has successfully completed the first major ste...
A non-Gaussian, flat-top laser beam profile, also called Mesa Beam Profile, supported by non spheric...
International audienceThe sensitivity of interferometric gravitational wave detectors is optimized, ...
A tunable Fabry-Perot interferometer (FPI) can be used as an optical band-pass filter. This type of ...
The sensitivity of interferometric gravitational wave detectors is optimized, in part, by balanced f...